Same as Fig. 6 but for the LMC. The tracks of Brott et al. (2011) are complemented with those of Köhler et al. (2015) for masses above 100 M_⊙. The left panel shows the 200 M_⊙ non-rotating tracks of Martins & Palacios (2022) in yellow. The right panels show models for an initial rotational velocity of 550 km s⁻¹. The red tracks are from Eggenberger et al. (2021). The bold part of the tracks is for a nitrogen mass fraction of greater than 0.0047. Open circles are stars in 30 Dor from Bestenlehner et al. (2011, 2020).